Flow Channels and the Generation of Alfvénic Turbulence Along Storm‐Time Inner Magnetospheric Field‐Lines-Reference-Cited by-同舟云学术

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Flow Channels and the Generation of Alfvénic Turbulence Along Storm‐Time Inner Magnetospheric Field‐Lines

Published:2022-12 Issue:23 Volume:49 Page:
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophysical Research Letters

Author:

Chaston Christopher C.¹^ORCID

Affiliation:

1. Space Sciences Laboratory University of California Berkeley CA USA

Funder

Heliophysics Division

National Science Foundation

U.S. Department of Energy

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2022GL101321

Reference55 articles.

1. Magnetotail waveguide: Fast and Alfvén waves in the plasma sheet boundary layer and lobe

2. The Space Physics Environment Data Analysis System (SPEDAS)

3. Statistical characteristics of bursty bulk flow events

4. Electron trapping and acceleration by kinetic Alfven waves in the inner magnetosphere

5. The Magnetic Electron Ion Spectrometer (MagEIS) Instruments Aboard the Radiation Belt Storm Probes (RBSP) Spacecraft

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Characteristics of plasma boundaries with large density gradients and their effects on Kelvin–Helmholtz instability;Frontiers in Astronomy and Space Sciences;2024-05-31

2. Electron Scattering, Transport and Energization by Alfvénic Turbulence in Earth's Outer Radiation Belt;Geophysical Research Letters;2023-06-30

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